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A small mass m is moved slowly from the ...

A small mass `m` is moved slowly from the surface of the earth to a height `h` above the surface. The work done (by an external agent) in doing this is

A

`mgh`, for all values of h

B

`mgh`, for `hlt ltR`

C

`1//2, mgR`, for `h=R`

D

`-1//2mgR`, for `h=R`

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To solve the problem of calculating the work done by an external agent in moving a small mass `m` from the surface of the Earth to a height `h`, we will follow these steps: ### Step 1: Understand the concept of gravitational potential energy The gravitational potential energy (U) at a distance `r` from the center of the Earth is given by the formula: \[ U = -\frac{G M m}{r} \] where: - \( G \) is the gravitational constant, - \( M \) is the mass of the Earth, - \( m \) is the mass of the object, - \( r \) is the distance from the center of the Earth. ### Step 2: Calculate the potential energy at the surface of the Earth At the surface of the Earth, the distance \( r \) is equal to the radius of the Earth \( R \): \[ U_1 = -\frac{G M m}{R} \] ### Step 3: Calculate the potential energy at height \( h \) At a height \( h \) above the surface, the distance from the center of the Earth becomes \( R + h \): \[ U_2 = -\frac{G M m}{R + h} \] ### Step 4: Calculate the work done by the external agent The work done (W) by the external agent in moving the mass from the surface to height \( h \) is the change in potential energy: \[ W = U_2 - U_1 \] Substituting the values from Steps 2 and 3: \[ W = \left(-\frac{G M m}{R + h}\right) - \left(-\frac{G M m}{R}\right) \] \[ W = \frac{G M m}{R} - \frac{G M m}{R + h} \] ### Step 5: Simplify the expression for work done Factoring out \( G M m \): \[ W = G M m \left(\frac{1}{R} - \frac{1}{R + h}\right) \] To combine the fractions: \[ W = G M m \left(\frac{(R + h) - R}{R(R + h)}\right) \] \[ W = G M m \left(\frac{h}{R(R + h)}\right) \] ### Step 6: Consider the case when \( h \) is very small compared to \( R \) If \( h \) is much smaller than \( R \) (i.e., \( h \ll R \)), we can approximate: \[ W \approx \frac{G M m h}{R^2} \] Since \( g = \frac{G M}{R^2} \), we can write: \[ W \approx mgh \] ### Step 7: Consider the case when \( h \) is equal to \( R \) If \( h = R \), substituting \( h \) into the work done expression: \[ W = G M m \left(\frac{R}{R^2}\right) = \frac{G M m}{R} \] This can be simplified further, but for practical purposes, we can conclude that the work done increases as \( h \) increases. ### Final Result Thus, the work done by an external agent in moving the mass \( m \) to height \( h \) is given by: \[ W = \frac{G M m h}{R(R + h)} \] And for small heights, it approximates to \( W \approx mgh \).

To solve the problem of calculating the work done by an external agent in moving a small mass `m` from the surface of the Earth to a height `h`, we will follow these steps: ### Step 1: Understand the concept of gravitational potential energy The gravitational potential energy (U) at a distance `r` from the center of the Earth is given by the formula: \[ U = -\frac{G M m}{r} \] where: - \( G \) is the gravitational constant, - \( M \) is the mass of the Earth, ...
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